Diagnosing the Accretion Flow Geometry of a Galactic Black Hole in Outburst with Chandra

Details Diagnosing the Accretion Flow Geometry of a Galactic Black Hole in Outburst with Chandra Diagnosing the Accretion Flow Geometry of a Galactic Black Hole in Outburst with Chandra

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cxo..prop.1174l&link_type=abstract

Chandra Proposal ID #04400392

Physics

Chandra Proposal Id #04400392

Scientific paper

We propose to study the accretion flow geometry of a Galactic black hole in outburst using the Chandra HETGS. Models for the accretion flow geometry in Galactic black holes make different predictions which can be tested with high resolution spectroscopy. We will build on the recent successes of this program -- including the detection of broad Fe K lines likely shaped by Doppler shifts and strong gravity, and narrow absorption lines in an outflowing disk atmosphere -- by obtaining spectra with improved sensitivity. We request a total of 200 ksec (4 obs. of 50 ksec; 1 ``fast'' TOO and 3 follow-ups) for this Chandra study. We will support these observations with simultaneous RXTE and Integral observations, and with radio and optical observations from approved programs around the globe.

Affiliated with

Also associated with

No associations

Rating

Diagnosing the Accretion Flow Geometry of a Galactic Black Hole in Outburst with Chandra does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Diagnosing the Accretion Flow Geometry of a Galactic Black Hole in Outburst with Chandra, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Diagnosing the Accretion Flow Geometry of a Galactic Black Hole in Outburst with Chandra will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1042381